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— CH. 1 · INTRODUCTION —

2012 VP113

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  • 2012 VP113 sits at the farthest known perihelion of any object in our Solar System. Its closest approach to the Sun never brings it within 80.5 astronomical units of our star. To put that in perspective, Pluto sits around 39 astronomical units from the Sun at its nearest. Scott Sheppard and Chad Trujillo, two American astronomers working at Cerro Tololo Inter-American Observatory in Chile, discovered it on the 5th of November 2012. They gave it a nickname almost immediately: Biden, after then-Vice President Joe Biden, because the letters "VP" appeared in its official designation. The discovery was not announced to the public until the 26th of March 2014, more than a year after it was first spotted. What is this distant, reddish world? Where exactly does it belong in the Solar System's family? And what does its orbit tell us about forces we have not yet seen?

  • The first observation came through NOAO's 4-meter Víctor M. Blanco Telescope at Cerro Tololo Inter-American Observatory. That initial detection, logged on the 5th of November 2012, put the object on the radar of a very small circle of scientists. For the months between discovery and public announcement, only two observatories tracked it: Cerro Tololo Inter-American Observatory, designated station 807, and Las Campanas Observatory, designated station 304. Carnegie's 6.5-meter Magellan telescope at Las Campanas Observatory in Chile was used to nail down its orbit and study its surface properties. Researchers also found the object hiding in precovery images dating as far back as September 2007, meaning it had been captured on camera years before anyone realized what they were looking at.

  • 2012 VP113 has an absolute magnitude of 4.05, a measure of intrinsic brightness that suggests it may be large enough to qualify as a dwarf planet. No one has measured its diameter or albedo directly. Assuming a moderate geometric albedo of 0.15, which is typical for trans-Neptunian objects, the diameter works out to around 450 kilometers. Astronomers expect it to be about half the size of Sedna, and roughly similar in size to Huya. Its surface has a moderately red color, produced by radiation acting on frozen water, methane, and carbon dioxide. That reddish tint is actually a chemical clue: it points toward formation in the gas-giant region of the Solar System rather than in the classical Kuiper belt, which tends to produce ultra-red colored objects. The Hubble Space Telescope is planned to image 2012 VP113 in 2026, an observation that should reveal whether it has any significantly sized moons.

  • 2012 VP113 holds a record that no other known Solar System body can claim: the farthest perihelion of any known minor planet or any other known object. Its closest approach to the Sun exceeds even Sedna's perihelion, though its aphelion is only about half of Sedna's. It qualifies as a sednoid, the second one ever discovered, defined by a semi-major axis beyond 150 astronomical units and a perihelion greater than 50. The giant planets sit too far inside to have any meaningful gravitational grip on it. Its last perihelion occurred within a couple of months of September 1979. Sheppard and Trujillo noticed that 2012 VP113 shares orbital traits with other extreme trans-Neptunian objects. In fact, all known Solar System bodies with semi-major axes over 150 and perihelia beyond Neptune cluster their arguments of perihelion near 340 degrees. That clustering led the two astronomers to propose that an undiscovered body, now referred to as Planet Nine, is steering these distant objects into similar orbits.

  • How 2012 VP113 wound up with a perihelion so far beyond the Kuiper belt is genuinely unknown. Several explanations have been proposed. A passing star could have pulled its orbit outward. A trans-Neptunian planet several times the mass of Earth, sitting hundreds of astronomical units from the Sun, could be responsible. The region beyond Pluto may even contain more than one such unseen planet. Scientists also consider the possibility that 2012 VP113 was captured from a completely different planetary system. The leading hypothesis, though, is that multiple gravitational interactions within the crowded open star cluster where the Sun formed gradually raised its perihelion to its current extreme distance. 2012 VP113 may also belong to a hypothesized region called the Hills cloud. The scarcity of objects with perihelia near 50 astronomical units is itself significant: it does not appear to be an accident of observation, and is referred to as the Kuiper cliff. That gap in the population is a puzzle astronomers are still working to explain.

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Common questions

Who discovered 2012 VP113 and when was it found?

2012 VP113 was discovered on the 5th of November 2012 by American astronomers Scott Sheppard and Chad Trujillo at Cerro Tololo Inter-American Observatory in Chile. The discovery was announced publicly on the 26th of March 2014.

Why is 2012 VP113 nicknamed Biden?

The discovery team nicknamed 2012 VP113 "Biden" because the letters "VP" appear in its official designation, and Joe Biden was serving as Vice President of the United States at the time of discovery.

How big is 2012 VP113?

The diameter of 2012 VP113 has not been directly measured, but based on an assumed geometric albedo of 0.15, typical for trans-Neptunian objects, it is estimated to be around 450 kilometers across. Its absolute magnitude of 4.05 suggests it may be large enough to be classified as a dwarf planet.

What makes 2012 VP113 a sednoid?

2012 VP113 is classified as a sednoid because its orbit never comes closer than 80.5 AU from the Sun, placing it well beyond the gravitational influence of the giant planets. It has a semi-major axis beyond 150 AU and a perihelion greater than 50 AU, making it only the second sednoid ever discovered.

What is the connection between 2012 VP113 and Planet Nine?

Discoverers Scott Sheppard and Chad Trujillo noted that the orbit of 2012 VP113 resembles those of other extreme trans-Neptunian objects, with all such known bodies clustering their arguments of perihelion near 340 degrees. They proposed that an undiscovered body, referred to as Planet Nine, may be gravitationally shepherding these distant objects into similar orbits.

What color is 2012 VP113 and what does that reveal about its origin?

2012 VP113 has a moderately red surface color caused by radiation acting on frozen water, methane, and carbon dioxide. This color is consistent with formation in the gas-giant region of the Solar System rather than the classical Kuiper belt, which is dominated by ultra-red objects.

All sources

19 references cited across the entry

  1. 3MPEC 2014-F40 : 2012 VP113IAU Minor Planet Center — 26 March 2014
  2. 4List of Known Trans-Neptunian ObjectsWm. Robert Johnston — 7 October 2018
  3. 52012 VP113 – SummaryAstDyS-2, Asteroids Dynamic Site
  4. 6JournalA Sedna-like body with a perihelion of 80 astronomical unitsChadwick A. Trujillo et al. — March 2014
  5. 7JournalDwarf planet stretches Solar System's edgeAlexandra Witze — 26 March 2014
  6. 10Beyond the Edge of the Solar System: The Inner Oort Cloud PopulationScott S. Sheppard — Department of Terrestrial Magnetism, Carnegie Institution for Science
  7. 11NewsA New Planetoid Reported in Far Reaches of Solar SystemKenneth Chang — 26 March 2014
  8. 14A second Sedna! What does it mean?Emily Lakdawalla — The Planetary Society — 26 March 2014
  9. 17JournalA Search For The Moons of Mid-Sized TNOsBenjamin Proudfoot — Space Telescope Science Institute — August 2025
  10. 18JournalExtreme trans-Neptunian objects and the Kozai mechanism: signalling the presence of trans-Plutonian planetsCarlos de la Fuente Marcos et al. — 1 September 2014
  11. 19JournalFlipping minor bodies: what comet 96P/Machholz 1 can tell us about the orbital evolution of extreme trans-Neptunian objects and the production of near-Earth objects on retrograde orbitsCarlos de la Fuente Marcos et al. — 11 January 2015